WSRT ZoA Perseus-Pisces. HI catalogue : J/MNRAS/460/923


Authors : Ramatsoku M. orcid , Verheijen M.A.W., Kraan-Korteweg R.C. (hide) , Verheijen M.A.W., Kraan-Korteweg R.C. et..al

Bibcode : 2016MNRAS.460..923R (ADS) (Simbad) (Objects) (hide)

CDS Keywords : Surveys; Clusters, galaxy; H I data; Radio lines
UAT : Surveys, Galaxy clusters, H I line emission, Radio astronomy

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Inserted into VizieR : 10-Nov-2017
Last modification : 16-Aug-2024

The WSRT ZoA Perseus-Pisces filament wide-field HI imaging survey. I. HI catalogue and atlas. (2016)

Keywords : atlases - catalogues - surveys - galaxies clusters: general - radio lines: galaxies

Abstract:We present results of a blind 21cm HI-line imaging survey of a galaxy overdensity located behind the Milky Way at l, b ~= 160{deg}, 0.5{deg}. The overdensity corresponds to a zone-of-avoidance crossing of the Perseus-Pisces Supercluster filament. Although it is known that this filament contains an X-ray galaxy cluster (3C 129) hosting two strong radio galaxies, little is known about galaxies associated with this potentially rich cluster because of the high Galactic dust extinction. We mapped a sky area of ~9.6 deg^2^ using the Westerbork Synthesis Radio Telescope in a hexagonal mosaic of 35 pointings observed for 12h each, in the radial velocity range cz=2400-16600km/s. The survey has a sensitivity of 0.36mJy/beam rms at a velocity resolution of 16.5km/s. ...(more)
Abstract: (hide)
Observations were carried out using the WSRT between 2012 August and November. We imaged a mosaic comprising 35 fields arranged in a hexagonal grid covering 9.6 deg^2^, each separated by {Delta}=0.5{deg}. The observational parameters for the 35 pointings are summarized in Table 1.


                
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